Posts by Collection

portfolio

publications

Black Hole-Halo Mass Relation from UNIONS Weak Lensing

Published in Astrophysical Journal Letters, 2024

Qinxun Li, Martin Kilbinger, Wentao Luo, Kai Wang, Huiyuan Wang, Anna Wittje, et al. "Black Hole-Halo Mass Relation from UNIONS Weak Lensing." Astrophysical Journal Letters, 2024.

DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints

Published in Physical Review D, 2025

DESI Collaboration, M. Abdul Karim, J. Aguilar, S. Ahlen, S. Alam, L. Allen, et al. "DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints." Physical Review D, 2025.

Contribution: I performed the consistency tests of BAO measurements and wrote Section III.C. I also made Figure 6 and 13, which show the BAO and SN distance measurements in comparison to various cosmological models.

talks

2022 PKU-DoA Undergraduate Astronomy Symposium: Subhalo Properties from SDSS Weak Lensing

Published:

This is a talk of 2022 PKU-DoA Undergraduate Astronomy Symposium. In this talk, I introduce my work on subhalo mass measurement from SDSS weak lensing. We use Luo et al. (2017) SDSS DR7 shape catalog to study subhaloes in Yang et al. (2006) group catalog. We find an unreported selection bias between host halo mass and separation between satellite galaxies and their central galaxies. We develop a weigting method to correct this bias. With a 2 free paramater model to describe excess surface density of subhalo, we fit the weighted lensing signal by MCMC. In this talk, I will first introduce galaxy-galaxy lensing method and subhalo density profile, then talk about the methods and main results of this work.

Cluster Seminar: Subhalo Properties in SDSS DR7 with Galaxy-galaxy Lensing

Published:

This is a talk of cluster seminar of Department of Astronomy, Umich. In this talk, I will focus on our recent work about subhalo properties in Yang et al. (2007) 's group catalog based on SDSS DR7. We devide satellite galaxies into different stellar mass and BCG-center separation bins, then measure the lensing signals around these satellites. We discover an unreported selection effect between separation and host halo mass and use a weighting method to correct it. With a 2 free paramater model to describe excess surface density of subhalo, we fit the weighted lensing signal by MCMC. In this talk, I will first introduce galaxy-galaxy lensing method and subhalo density profile, then talk about the methods and main results of this work.

Introduction to Modern Cosmology

Published:

Invited talk at the Southern University of Science & Technology 2nd Student Physics & Mathametics Workshop.